Answer:
B. 0.1 meters/second/second in the same direction of travel.
Explanation:
Acceleration is the rate of change of velocity. Acceleration is a vector quantity.
a=Δv/Δt
=(v₂-v₁)/(t₂-t₁)
v₁=4 m/s
v₂=6 m/s
t₁=0 s
t₂=20 s
a=(6m/s-4m/s)/(20s-0)
= 0.1 m/s² in the same direction of travel.
Therefore acceleration =0.1 meters/second/second in the same direction of travel.
Hello!
Answer:
Regular physical activity in life improves strength and endurance, helps build healthy bones and muscles, helps control weight, reduces anxiety and stress, increases self-esteem, and it can improve blood pressure and cholesterol levels.
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<u>Hope this help<3</u>
If an object is moving and has velocity it has kinetic energy. the kinetic energy of an object is the energy that it possesses due to its motion.
In my work I used the formula for kinetic energy to answer your question. Hope this helps.
Answer:
![r=97.22x10^{3} m](https://tex.z-dn.net/?f=r%3D97.22x10%5E%7B3%7D%20m)
Explanation:
Using the angular formulas can determine the radius using both values neutron star and the the knowing star so
![L=I*w](https://tex.z-dn.net/?f=L%3DI%2Aw)
![L_{1}=I_{1}*w_{1}=L_{2}=I_{2}*w_{2}](https://tex.z-dn.net/?f=L_%7B1%7D%3DI_%7B1%7D%2Aw_%7B1%7D%3DL_%7B2%7D%3DI_%7B2%7D%2Aw_%7B2%7D)
![I_{1}*w_{1}=I_{2}*w_{2}](https://tex.z-dn.net/?f=I_%7B1%7D%2Aw_%7B1%7D%3DI_%7B2%7D%2Aw_%7B2%7D)
I=Inertia of the star
w=angular velocity
![I=\frac{2*m*r^{2}}{5}](https://tex.z-dn.net/?f=I%3D%5Cfrac%7B2%2Am%2Ar%5E%7B2%7D%7D%7B5%7D)
![w=\frac{2\pi}{t}](https://tex.z-dn.net/?f=w%3D%5Cfrac%7B2%5Cpi%7D%7Bt%7D)
Notice the angular velocity determinate by the time and the Inertia have the radius value so
![\frac{2}{5}*m*r_{sn}^{2}*\frac{2\pi }{t_{1}}=\frac{2}{5}*m*r_{s}^{2}*\frac{2\pi }{t_{2}}](https://tex.z-dn.net/?f=%5Cfrac%7B2%7D%7B5%7D%2Am%2Ar_%7Bsn%7D%5E%7B2%7D%2A%5Cfrac%7B2%5Cpi%20%7D%7Bt_%7B1%7D%7D%3D%5Cfrac%7B2%7D%7B5%7D%2Am%2Ar_%7Bs%7D%5E%7B2%7D%2A%5Cfrac%7B2%5Cpi%20%7D%7Bt_%7B2%7D%7D)
![r_{sn}^{2}*\frac{1}{t_{1}}=r_{s}^{2}*\frac{1}{t_{2}}](https://tex.z-dn.net/?f=r_%7Bsn%7D%5E%7B2%7D%2A%5Cfrac%7B1%7D%7Bt_%7B1%7D%7D%3Dr_%7Bs%7D%5E%7B2%7D%2A%5Cfrac%7B1%7D%7Bt_%7B2%7D%7D)
![r_{sn}^{2}=r_{s}^{2}*\frac{t_{1}}{t_{2}}](https://tex.z-dn.net/?f=r_%7Bsn%7D%5E%7B2%7D%3Dr_%7Bs%7D%5E%7B2%7D%2A%5Cfrac%7Bt_%7B1%7D%7D%7Bt_%7B2%7D%7D)
![t_{1}=0.2s\\t_{2}=30day*\frac{24hr}{1day}*\frac{60minute}{1hr}*\frac{60seg}{1minute}=2.592x10^{6}s](https://tex.z-dn.net/?f=t_%7B1%7D%3D0.2s%5C%5Ct_%7B2%7D%3D30day%2A%5Cfrac%7B24hr%7D%7B1day%7D%2A%5Cfrac%7B60minute%7D%7B1hr%7D%2A%5Cfrac%7B60seg%7D%7B1minute%7D%3D2.592x10%5E%7B6%7Ds)
![r_{sn}=3.5x10^{8}m*\sqrt{\frac{0.2s}{2.592x^{6}s}}](https://tex.z-dn.net/?f=r_%7Bsn%7D%3D3.5x10%5E%7B8%7Dm%2A%5Csqrt%7B%5Cfrac%7B0.2s%7D%7B2.592x%5E%7B6%7Ds%7D%7D)
![r_{sn}=97.22x10^{3} m](https://tex.z-dn.net/?f=r_%7Bsn%7D%3D97.22x10%5E%7B3%7D%20m)
Answer:
The reason why first impressions are so important is that they last well beyond that moment. This is thanks to something called the primacy effect, which means that when someone experiences something before other things in a sequence, they remember that first thing more.